{"arxiv_id":"astro-ph/0112051","incoming":{"papers":3,"sentences":3,"groups":[{"kind":"data_used","label":"Uses its data or values","papers":1,"sentences":1,"quotes":[{"arxiv_id":"2503.07725","title":"Measuring Type Ia Supernova Angular-Diameter Distances with Intensity Interferometry","url":"/paper/2503.07725","section":"Introduction","sentence":"SNe Ia have a rate of $r_v = 2.43 ×10^-5 SNe yr^-1 Mpc^-3 h^3_ 70$ [ref] and on average reach a peak absolute magnitude of $B =-19.13 - 5log(h_70)$ [ref] .","intent_p":1.0,"contests_p":null}]},{"kind":"background","label":"Cites it as background","papers":1,"sentences":1,"quotes":[{"arxiv_id":"2608.20781","title":"Pandora cluster Lensing, AGN, and Transient Exploration (PLATE) from JWST Multi-Epoch Imaging. I. Discovery of a type II supernova candidate in a spiral galaxy at $z=0.7$","url":"/paper/2608.20781","section":"Introduction","sentence":"Historically, they were divided into SNe IIP, which exhibit a roughly 100-day phase of nearly constant optical luminosity, and SNe IIL, whose light curves decline more rapidly and approximately linearly in magnitude after peak luminosity [ref] .","intent_p":1.0,"contests_p":null}]}],"unlabelled_sentences":1},"outgoing":{"papers":0,"sentences":0,"groups":[],"unlabelled_sentences":0},"claims":[],"thresholds":{"intent_p":0.8,"supports_p":0.95,"contests_p":0.7},"method":"Citing sentences come from each paper's LaTeX source; every \\cite marks the sentence and the works it cites. Pith's classifier typed each sentence. A label is shown at intent probability 0.8 or more (0.95 for support), a contest at 0.7 or more. Measured accuracy against two blind model families is at https://pith.science/accuracy. The quoted sentences are the citing authors' own.","held_up":null,"_links":{"html":"https://pith.science/paper/astro-ph/0112051"}}